**Table 3:** Summary of the results of the data analysis. The columns denote, respectively: sequence number of the observation, date of observation, Heliocentric Julian date, measured longitudinal component of magnetic field strength (integrated over the stellar disk) with 1 $\sigma$ errors, velocity of the minimum, and first moment of the Stokes I line profile, both with 1 $\sigma$ errors, for all observed targets arranged in the same order as in Table 2.
$\begin{displaymath}\fontsize{26}{28}\selectfont \begin{tabular}{@{ }r@{$\:\:\:$}... ...456 & $-$118&104 & $-$47&1 & $-$2.0&0.3\\ \hline \end{tabular}\end{displaymath}$

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